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Magnetic Accretion Model for the Activities of Very Young Stars

Published online by Cambridge University Press:  12 April 2016

Yutaka Uchida
Yutaka Uchida*
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo, Japan

Abstract:

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A magnetodynamic model is proposed to interpret the observed inflow-outflow-X-ray emitting region complex in the atmospheres of T Tau stars.

Type
Session IV: Theoretical Aspects
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 625 - 627
Copyright
Copyright © Reidel 1983

References

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